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Observational Constraints on Higher Order Clustering up to z ≃ 1

  • Authors: István Szapudi, Marc Postman, Tod R. Lauer, and William Oegerle

Szapudi et al. 2001 The Astrophysical Journal 548 114.

  • Provider: AAS Journals

Caption: Fig. 2.

Three‐point correlation function z, displayed in terms of the hierarchical term ﹩w( 1) w( 2) +w( 2) w( 3) +w( 3) w( 1) ﹩. The long‐dashed lines show the limits that were used to exclude outliers in the ﹩\chi ^{2}﹩ fit for the parameters of the general third‐order connected expansion. Dotted lines display the results from the counts‐in‐cells analysis, while short‐dashed lines show ﹩q_{3}﹩ from the ﹩\chi ^{2}﹩ fit.

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